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cloelike is the likelihood module for Euclid primary observables, interfacing with cloelib.

✨ Features

🔹 loglike calculation for Euclid primary probes – currently supporting 3×2pt and spectroscopic galaxy clustering full-shape and BAOs

🔹 Modular design – Mix-and-match photometric probes (WL, GCph, GGL) using composable mixin classes

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📋 Available Likelihoods

Class	Observable
EuclidLikelihood_WL	Weak Lensing (WL) angular power spectra
EuclidLikelihood_GCph	Photometric Galaxy Clustering (GCph) angular power spectra
EuclidLikelihood_GGL	Galaxy–Galaxy Lensing (GGL) angular power spectra
EuclidLikelihood_3x2pt	3×2pt (WL + GCph + GGL) combined
EuclidLikelihood_2x2pt	2×2pt (WL + GGL) combined
EuclidLikelihood_GCspectro_Pls	Spectroscopic Galaxy Clustering (GCspectro) power spectrum multipoles
EuclidLikelihood_BAO	Baryon Acoustic Oscillations (BAO)

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🤝 Contributors

This project follows the all-contributors specification. Contributions of any kind are welcome!

Guadalupe Cañas-Herrera 💻 🚧 🤔 🐛 🖋 🔣 📖 🚇 📆 💬 ⚠️ 📢 👀	AndreaPezzotta 💻 🚧 🤔 🐛 🖋 🔣 📖 📢 👀	Pedro Carrilho 💻 🚧 🤔 🐛 🖋 🔣 📖 📢	itutusaus 👀	Marco Bonici 👀	Santiago Casas 🤔 👀	Chiara Moretti 💻 🤔 🚧 🖋 🔣 📢 🐛
Nicolas Tessore 👀 🤔	Davide Sciotti 💻 🐛 🤔	Zahra Baghkhani 💻 📖	Jip de Buck 🐛	KlaraBertmann 💻	Peter L. Taylor 💻 🤔	Felicitas Keil 🐛 💻
Martin Kärcher 💻 🤔

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⚖️ License

This project is licensed under the MIT License.